LBA fringe test
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From: <Chris.Phillips_at_email.protected>
Date: Fri, 19 Sep 2014 09:35:06 +0000
Hi all
Sorry I meant to send this email earlier.
For this session the main Oz fringe test are rolled into the main experiment (except v490c).
The vcxcx experiments are for fringe testing with Hart (there are no good 22 gHz source suitable for Hart, Parkes and Ceduna).
So for all experiments, start with the main experiment schedule which starts at the time of the vcxcx experiment. A subset of telescopes (probably ATCA and Mopra) will then fringe test with Hart.
For v490 there are 3 vc249 experiments (a,b,c) there are for the 2 frequencies (a and b) and then c is for with Hart.
I hope this makes sense!
Regards
Chris
Received on 2014-09-19 19:35:07
Date: Fri, 19 Sep 2014 09:35:06 +0000
Hi all
Sorry I meant to send this email earlier.
For this session the main Oz fringe test are rolled into the main experiment (except v490c).
The vcxcx experiments are for fringe testing with Hart (there are no good 22 gHz source suitable for Hart, Parkes and Ceduna).
So for all experiments, start with the main experiment schedule which starts at the time of the vcxcx experiment. A subset of telescopes (probably ATCA and Mopra) will then fringe test with Hart.
For v490 there are 3 vc249 experiments (a,b,c) there are for the 2 frequencies (a and b) and then c is for with Hart.
I hope this makes sense!
Regards
Chris
Received on 2014-09-19 19:35:07